The Toronto Magnetic and Meteorological Observatory building from which the 1882 transit of Venus (ToV) was supposed to be observed survives, although it was moved to its present location subsequent to 1882. The observatory tower was built to house the high quality 152mm O.G. Thomas Cooke refractor commissioned for the ToV. The telescope also survives, and is in the collections of the Canada Science and Technology Museum in Ottawa.

This is a fine posthumous copper-plate portrait of the Rev'd Dr. Edmund Halley (1656-1742), the second Astronomer Royal (1720-1742). Halley is in many ways the father of the Transit of Venus enterprise, for he is the one who realized the practicality of using ToV observations to determine the Sun-Earth distance (the Astronomical Unit, AU), who devised a method for doing so (the so-called Halleyan Method), and who encouraged the mounting of a 1769 ToV campaign to that end, although he himself was unlikely to live to take part, or see the results.

Professor John Winthrop, Harvard College’s Hollisian Professor of Mathematics and Philosophy, successfully observed the 1761 transit from "Venus Hill", now thought to be somewhere in the vicinity of St. John's (Kenmount Hill?).

Thomas Wright, Deputy Surveyor of the Northern District of America, observed the 1769 transit of Venus successfully from Île aux Coudres in the Saint Lawrence River, Quebec. The quality of his observations was praised by the Astronomer Royal, the Rev'd Neville Maskelyne, in the pages of the Royal Society's Philosophical Transactions. Unbeknownst to both Wright and Maskelyne, the Île aux Coudres transit station was slap in the middle of an ancient meteorite impact site, the Charlevoix crater. This drawing is a recreation of the island site in 1769.